activity
19952026
most citedSelf-consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence

610 citations · 6.3k across the 100 of their papers we have counts for

collaborators
Showing 2010Show all

10 papers · 1 filter

astro-ph.SR2010★ 3 cited

Stellar Imager (SI): developing and testing a predictive dynamo model for the Sun by imaging other stars

Kenneth G. Carpenter, Carolus J. Schrijver, Margarita Karovska +39

The Stellar Imager mission concept is a space-based UV/Optical interferometer designed to resolve surface magnetic activity and subsurface structure and flows of a population of Su…

astro-ph.SR2010★ 3 cited

Science Objectives for an X-Ray Microcalorimeter Observing the Sun

J. Martin Laming, J. Adams, D. Alexander +57

We present the science case for a broadband X-ray imager with high-resolution spectroscopy, including simulations of X-ray spectral diagnostics of both active regions and solar fla…

astro-ph.SR2010

Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind Acceleration

S. R. Cranmer, J. L. Kohl, D. Alexander +21

Understanding the physical processes responsible for accelerating the solar wind requires detailed measurements of the collisionless plasma in the extended solar corona. Some key c…

astro-ph.SR2010★ 80 cited

Can the Solar Wind be Driven by Magnetic Reconnection in the Sun's Magnetic Carpet?

Steven R. Cranmer, Adriaan A. van Ballegooijen

The physical processes that heat the solar corona and accelerate the solar wind remain unknown after many years of study. Some have suggested that the wind is driven by waves and t…

astro-ph.SR2010★ 77 cited

Self Consistent Models of the Solar Wind

Steven R. Cranmer

The origins of the hot solar corona and the supersonically expanding solar wind are still the subject of much debate. This paper summarizes some of the essential ingredients of rea…

astro-ph.SR2010★ 2 cited

The Tale of Two Minima and a Solar Cycle in Between: An Ongoing Fast Solar Wind Investigation

M. P. Miralles, S. R. Cranmer, A. V. Panasyuk +1

We have measured the physical properties of polar coronal holes from the minimum activity phase of solar cycle 23 (1996-1997) to the present minimum of solar cycle 24 (2007-2009) u…